恒星核合成的全新诠释

Physicists¹ at the University of York have revealed a new understanding of nucleosynthesis in stars, providing insight into the role massive stars play in the evolution of the Milky² Way and the origins of the Solar System. Radioactive aluminium³ (aluminium-26, or Al26) is an element that emits gamma radiation through its decay enabling astronomers⁴ to image its location in our galaxy⁵. Studying how Al26 is created in massive stars, scientists have distinguished⁶ between previously⁷ conflicting assumptions about its rate of production by nuclear fusion⁸.

 

Funded by the Science and Technologies Research Council (STFC), scientists measured the fusion of helium and sodium⁹ at two separate particle accelerators in Canada and Denmark, and the rate of production of Al26 was determined¹⁰ to within a factor of two. An improvement on previous experiments where there was disagreement of around a factor of 100 between measurements, this outcome removes dispute about the effect of sodium fusion on the rate of aluminium production.

 

Al26 is known for its relatively¹¹ short lifespan (in astrophysical terms), decaying in around 1 million years, compared with the lifetime of massive stars of about 19 million years. This means we are now able to better understand gamma radiation maps of the galaxy, observed by space telescopes such as INTEGRAL and COMPTEL, and deduce a more accurate picture of recent activities of massive stars in the galaxy. 

 

Evidence of Al26 decay observed in meteorites¹² and pre-solar grains also suggests that material from massive stars contaminated the gas cloud from which the Solar System formed, providing insight into its early existence.

 

Dr Alison Laird, Reader in the University of York's Department of Physics and lead author on one of the two research papers, said: "This research highlights clear and unambiguous evidence from gamma-ray observations of the galaxy that nucleosynthesis is happening in stars. By pinning down the production rate of radioactive aluminium, we will be able to interpret and understand these observations.

 

"Now we better understand the processes within stars that drive aluminium production, we pave the way for more detailed¹³ and thorough research into how massive stars affect our galaxy and the origins of our Solar System."

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